Partitioning (clustering) of the data into k clusters “around
  medoids”, a more robust version of K-means.
pam(x, k, diss = inherits(x, "dist"),
    metric = c("euclidean", "manhattan"), 
    medoids = NULL, stand = FALSE, cluster.only = FALSE,
    do.swap = TRUE,
    keep.diss = !diss && !cluster.only && n < 100,
    keep.data = !diss && !cluster.only,
    pamonce = FALSE, trace.lev = 0)data matrix or data frame, or dissimilarity matrix or object,
    depending on the value of the diss argument.
In case of a matrix or data frame, each row corresponds to an
    observation, and each column corresponds to a variable.  All
    variables must be numeric.  Missing values (NAs)
    are allowed---as long as every pair of observations has at
    least one case not missing.
In case of a dissimilarity matrix, x is typically the output
    of daisy or dist.  Also a vector of
    length n*(n-1)/2 is allowed (where n is the number of observations),
    and will be interpreted in the same way as the output of the
    above-mentioned functions. Missing values (NAs) are
    not allowed.
positive integer specifying the number of clusters, less than the number of observations.
logical flag: if TRUE (default for dist or
    dissimilarity objects), then x will be considered as a
    dissimilarity matrix.  If FALSE, then x will be considered as
    a matrix of observations by variables.
character string specifying the metric to be used for calculating
    dissimilarities between observations.
    The currently available options are "euclidean" and
    "manhattan".  Euclidean distances are root sum-of-squares of
    differences, and manhattan distances are the sum of absolute
    differences.  If x is already a dissimilarity matrix, then
    this argument will be ignored.
NULL (default) or length-k vector of integer
    indices (in 1:n) specifying initial medoids instead of using
    the ‘build’ algorithm.
logical; if true, the measurements in x are
    standardized before calculating the dissimilarities.  Measurements
    are standardized for each variable (column), by subtracting the
    variable's mean value and dividing by the variable's mean absolute
    deviation.  If x is already a dissimilarity matrix, then this
    argument will be ignored.
logical; if true, only the clustering will be computed and returned, see details.
logical indicating if the swap phase should
    happen. The default, TRUE, correspond to the
    original algorithm.  On the other hand, the swap phase is
    much more computer intensive than the build one for large
    \(n\), so can be skipped by do.swap = FALSE.
logicals indicating if the dissimilarities
    and/or input data x should be kept in the result.  Setting
    these to FALSE can give much smaller results and hence even save
    memory allocation time.
logical or integer in 0:5 specifying algorithmic
    short cuts as proposed by Reynolds et al. (2006), and
    Schubert and Rousseeuw (2019) see below.
integer specifying a trace level for printing
    diagnostics during the build and swap phase of the algorithm.
    Default 0 does not print anything; higher values print
    increasingly more.
an object of class "pam" representing the clustering.  See
  ?pam.object for details.
The basic pam algorithm is fully described in chapter 2 of
  Kaufman and Rousseeuw(1990).  Compared to the k-means approach in kmeans, the
  function pam has the following features: (a) it also accepts a
  dissimilarity matrix; (b) it is more robust because it minimizes a sum
  of dissimilarities instead of a sum of squared euclidean distances;
  (c) it provides a novel graphical display, the silhouette plot (see
  plot.partition) (d) it allows to select the number of clusters
  using mean(silhouette(pr)[, "sil_width"]) on the result
  pr <- pam(..), or directly its component
  pr$silinfo$avg.width, see also pam.object.
When cluster.only is true, the result is simply a (possibly
  named) integer vector specifying the clustering, i.e.,
  pam(x,k, cluster.only=TRUE) is the same as 
  pam(x,k)$clustering but computed more efficiently.
The pam-algorithm is based on the search for k
  representative objects or medoids among the observations of the
  dataset.  These observations should represent the structure of the
  data.  After finding a set of k medoids, k clusters are
  constructed by assigning each observation to the nearest medoid.  The
  goal is to find k representative objects which minimize the sum
  of the dissimilarities of the observations to their closest
  representative object.
By default, when medoids are not specified, the algorithm first
  looks for a good initial set of medoids (this is called the
  build phase).  Then it finds a local minimum for the
  objective function, that is, a solution such that there is no single
  switch of an observation with a medoid that will decrease the
  objective (this is called the swap phase).
When the medoids are specified, their order does not
  matter; in general, the algorithms have been designed to not depend on
  the order of the observations.
The pamonce option, new in cluster 1.14.2 (Jan. 2012), has been
  proposed by Matthias Studer, University of Geneva, based on the
  findings by Reynolds et al. (2006) and was extended by Erich Schubert,
  TU Dortmund, with the FastPAM optimizations.
The default FALSE (or integer 0) corresponds to the
  original “swap” algorithm, whereas pamonce = 1 (or
  TRUE), corresponds to the first proposal .... 
  and pamonce = 2 additionally implements the second proposal as
  well. 
The key ideas of FastPAM (Schubert and Rousseeuw, 2019) are implemented except for the linear approximate build as follows:
pamonce = 3:reduces the runtime by a factor of O(k) by exploiting that points cannot be closest to all current medoids at the same time.
pamonce = 4:additionally allows executing multiple swaps per iteration, usually reducing the number of iterations.
pamonce = 5:adds minor optimizations copied from the
      pamonce = 2 approach, and is expected to be the fastest
      variant.
Reynolds, A., Richards, G., de la Iglesia, B. and Rayward-Smith, V. (1992) Clustering rules: A comparison of partitioning and hierarchical clustering algorithms; Journal of Mathematical Modelling and Algorithms 5, 475--504. 10.1007/s10852-005-9022-1.
Erich Schubert and Peter J. Rousseeuw (2019) Faster k-Medoids Clustering: Improving the PAM, CLARA, and CLARANS Algorithms; Preprint, (https://arxiv.org/abs/1810.05691).
agnes for background and references;
  pam.object, clara, daisy,
  partition.object, plot.partition,
  dist.
# NOT RUN {
## generate 25 objects, divided into 2 clusters.
x <- rbind(cbind(rnorm(10,0,0.5), rnorm(10,0,0.5)),
           cbind(rnorm(15,5,0.5), rnorm(15,5,0.5)))
pamx <- pam(x, 2)
pamx # Medoids: '7' and '25' ...
summary(pamx)
plot(pamx)
## use obs. 1 & 16 as starting medoids -- same result (typically)
(p2m <- pam(x, 2, medoids = c(1,16)))
## no _build_ *and* no _swap_ phase: just cluster all obs. around (1, 16):
p2.s <- pam(x, 2, medoids = c(1,16), do.swap = FALSE)
p2.s
p3m <- pam(x, 3, trace = 2)
## rather stupid initial medoids:
(p3m. <- pam(x, 3, medoids = 3:1, trace = 1))
# }
# NOT RUN {
pam(daisy(x, metric = "manhattan"), 2, diss = TRUE)
data(ruspini)
## Plot similar to Figure 4 in Stryuf et al (1996)
# }
# NOT RUN {
plot(pam(ruspini, 4), ask = TRUE)
# }
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